Fine structure of the interplanetary shock front according to measurements of the ion flux of the solar wind with high time resolution

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F17%3A10371307" target="_blank" >RIV/00216208:11320/17:10371307 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1134/S0010952517010038" target="_blank" >http://dx.doi.org/10.1134/S0010952517010038</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1134/S0010952517010038" target="_blank" >10.1134/S0010952517010038</a>

Result language
angličtina
Original language name
Fine structure of the interplanetary shock front according to measurements of the ion flux of the solar wind with high time resolution
Original language description
According to the data of the BMSW/SPEKTR-R instrument, which measured the density and velocity of solar wind plasma with a record time resolution, up to similar to 3 x10(-2) s, the structure of the front of interplanetary shocks has been investigated. The results of these first investigations were compared with the results of studying the structure of the bow shocks obtained in previous years. A comparison has shown that the quasi-stationary (averaged over the rapid oscillations) distribution of plasma behind the interplanetary shock front was significantly more inhomogeneous than that behind the bow-shock front, i.e., in the magnetosheath. It has also been shown that, to determine the size of internal structures of the fronts of quasi-perpendicular (theta(BN) > 45A degrees) shocks, one could use the magnetic field magnitude, the proton density, and the proton flux of the solar wind on almost equal terms. A comparison of low Mach (De (D) < 2), low beta (beta(1) < 1) fronts of interplanetary and bow shocks has shown that the dispersion of oblique magnetosonic waves plays an essential role in their formation.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10305 - Fluids and plasma physics (including surface physics)

Project
<a href="/en/project/GA16-04956S" target="_blank" >GA16-04956S: Solar wind as a natural laboratory: structure, turbulence, and shocks.</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical
Cosmic Research (English translation of Kosimicheskie Issledovaniya)
ISSN
0010-9525
e-ISSN
—
Volume of the periodical
55
Issue of the periodical within the volume
1
Country of publishing house
RU - RUSSIAN FEDERATION
Number of pages
16
Pages from-to
30-45
UT code for WoS article
000394182700004
EID of the result in the Scopus database
2-s2.0-85011932298

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